Gravity Wave Activity in the Stratosphere and Mesosphere at the South Pole (2024)

    Collins, R. L. / Gardner, C. S. / Committee on Space Research; Scientific Commission C

    • Neue Suche nach: Collins, R. L.
    • Neue Suche nach: Gardner, C. S.
    • Neue Suche nach: Committee on Space Research; Scientific Commission C
    • Neue Suche nach: Collins, R. L.
    • Neue Suche nach: Gardner, C. S.
    • Neue Suche nach: Hernandez, G.
    • Neue Suche nach: Smith, R. W.
    • Neue Suche nach: Committee on Space Research; Scientific Commission C

    In: Southern hemisphere upper atmosphere and ionosphere 5 ; 81-90 ; 1995

    • ISBN:

      0080426255

    • ISSN:

      0273-1177

    • Aufsatz (Konferenz) / Print

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    • Titel:

      Gravity Wave Activity in the Stratosphere and Mesosphere at the South Pole

    • Beteiligte:

      Collins, R. L. ( Autor:in ) / Gardner, C. S. ( Autor:in ) / Hernandez, G. / Smith, R. W. / Committee on Space Research; Scientific Commission C

    • Kongress:

      Meeting C.3; 30th Scientific assembly, Southern hemisphere upper atmosphere and ionosphere ; 1994 ; Hamburg; Germany

    • Erschienen in:

      Southern hemisphere upper atmosphere and ionosphere , 5 ; 81-90

      ADVANCES IN SPACE RESEARCH -OXFORD- ; 16, 5 ; 81-90

    • Verlag:

      Pergamon

      • Neue Suche nach: Pergamon
    • Erscheinungsdatum:

      01.01.1995

    • Format / Umfang:

      10 pages

    • ISBN:

      0080426255

    • ISSN:

      0273-1177

    • Medientyp:

      Aufsatz (Konferenz)

    • Format:

      Print

    • Sprache:

      Englisch

    • Schlagwörter:

      COSPAR , southern hemisphere , upper atmosphere , ionosphere

    • Datenquelle:

      British Library Conference Proceedings

    © Metadata Copyright the British Library Board and other contributors. All rights reserved.

    Inhaltsverzeichnis Konferenzband

    Die Inhaltsverzeichnisse werden automatisch erzeugt und basieren auf den im Index des TIB-Portals verfügbaren Einzelnachweisen der enthaltenen Beiträge. Die Anzeige der Inhaltsverzeichnisse kann daher unvollständig oder lückenhaft sein.

    3

    Thermospheric Dynamics in the Southern Polar Region

    Rees, D. / Hernandez, G. / Smith, R. W. / Committee on Space Research; Scientific Commission C et al. | 1995

    Gedruckte Ausgabe

    17

    Optical Interferometric Observations of 630-nm Intensities, Thermospheric Winds and Temperatures Near the Geomagnetic Equator

    Meriwether, J. W. / Biondi, M. A. / Committee on Space Research; Scientific Commission C et al. | 1995

    Gedruckte Ausgabe

    27

    Observations of Thermospheric Neutral Winds and Temperatures at Cachoeira Paulista (23S, 45W) During a Geomagnetic Storm

    fa*gundes, P. R. / Sahai, Y. / Bittencourt, J. A. / Takahashi, H. / Committee on Space Research; Scientific Commission C et al. | 1995

    Gedruckte Ausgabe

    31

    Upper Thermospheric Temperatures at South Pole

    Smith, R. W. / Hernandez, G. / Committee on Space Research; Scientific Commission C et al. | 1995

    Gedruckte Ausgabe

    41

    Thermospheric Horizontal Winds Above Mawson, Antarctica

    Conde, M. / Dyson, P. L. / Committee on Space Research; Scientific Commission C et al. | 1995

    Gedruckte Ausgabe

    53

    Southern Hemisphere Dynamics Observed by WINDII: The Wind Imaging Interferometer on the UARS Mission

    Shepherd, G. G. / McLandress, C. / Committee on Space Research; Scientific Commission C et al. | 1995

    Gedruckte Ausgabe

    61

    What Can Be Learned from Rotational Temperatures Derived from Ground-Based Airglow Observations about the Aeronomy of the Southern Hemisphere

    Scheer, J. / Committee on Space Research; Scientific Commission C et al. | 1995

    Gedruckte Ausgabe

    71

    Antarctic High-latitude Mesospheric Dynamics

    Hernandez, G. / Smith, R. W. / Fraser, G. J. / Committee on Space Research; Scientific Commission C et al. | 1995

    Gedruckte Ausgabe

    81

    Gravity Wave Activity in the Stratosphere and Mesosphere at the South Pole

    Collins, R. L. / Gardner, C. S. / Committee on Space Research; Scientific Commission C et al. | 1995

    Gedruckte Ausgabe

    91

    Ground Based Radar Investigation of the Antarctic Mesosphere

    Von Biel, H. A. / Committee on Space Research; Scientific Commission C et al. | 1995

    Gedruckte Ausgabe

    99

    Modelling Studies of North-South Differences in the Ionosphere at Mid Latitudes

    Balan, N. / Bailey, G. J. / Titheridge, J. E. / Committee on Space Research; Scientific Commission C et al. | 1995

    Gedruckte Ausgabe

    103

    Radio Studies of the Southern Hemisphere High-latitude Ionosphere

    Dyson, P. L. / Parkinson, M. L. / Quach, A. D. / Smith, P. R. / Committee on Space Research; Scientific Commission C et al. | 1995

    Gedruckte Ausgabe

    113

    Observations of Gravity Waves Associated with Mid-Latitude Spread-F

    Dyson, P. L. / Johnston, D. L. / Scali, J. L. / Committee on Space Research; Scientific Commission C et al. | 1995

    Gedruckte Ausgabe

    117

    Relationship Between Geneation of Equatorial F-Region Plasma Bubbles and Thermospheric Dynamics

    fa*gundes, P. R. / Sahai, Y. / Bittencourt, I. A. / Takahashi, H. / Committee on Space Research; Scientific Commission C et al. | 1995

    Gedruckte Ausgabe

    121

    Geomagnetic Pulsations in the Ionosphere

    Menk, F. W. / Marshall, R. A. / Waters, C. L. / Dunlop, I. S. / Committee on Space Research; Scientific Commission C et al. | 1995

    Gedruckte Ausgabe

    131

    Global Electrodynamics from Superpressure Balloons

    Holzworth, R. H. / Hu, H. / Committee on Space Research; Scientific Commission C et al. | 1995

    Gedruckte Ausgabe

    141

    Upper Atmosphere Research at INPE

    Clemesha, B. R. / Takahashi, H. / Committee on Space Research; Scientific Commission C et al. | 1995

    Gedruckte Ausgabe

    151

    Australian Antarctic Middle and Upper Atmospheric Physics - A New Direction

    Morris, R. J. / Monselesan, D. P. / Klekociuk, A. R. / Committee on Space Research; Scientific Commission C et al. | 1995

    Gedruckte Ausgabe

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    Gravity Wave Activity in the Stratosphere and Mesosphere at the South Pole (2024)

    FAQs

    What is the gravity wave in the atmosphere? ›

    In a gravity wave, the upward moving region is the most favorable region for cloud development and the sinking region favorable for clear skies. That is why you may see rows of clouds and clear areas between the rows of clouds. A gravity wave is nothing more than a wave moving through a stable layer of the atmosphere.

    What are the gravity waves in the thermosphere? ›

    Gravity waves in the atmosphere are the waves with gravity and buoyancy force as the restoring forces. Gravity waves will significantly impact the Mesosphere Lower / Thermosphere (MLT), and the breaking of gravity waves is the key factor to cause the cool summer and warm winter in the Mesopause region.

    What are internal gravity waves in the atmosphere? ›

    Internal gravity waves are waves occurring in the interior of a stratified fluid, with buoyancy providing the restoring force which opposes vertical displacements. Such waves are ubiquitous in the atmosphere and ocean and are the internal counterpart to the familiar surface gravity waves.

    What causes gravity wave clouds? ›

    They form when air is forced upward by hills or mountains into a layer of stable air in the atmosphere. Gravity causes the air to fall back down, and it begins to oscillate, creating a ripple effect. Wind flowing over the Rocky Mountains, for example, can create gravity waves that are felt as turbulence on an airplane.

    How do gravity waves affect us? ›

    From even the distance of the nearest star, gravitational waves would pass through us almost completely unnoticed. Although these ripples in spacetime carry more energy than any other cataclysmic event, the interactions are so weak that they barely affect us.

    Has there ever been a gravity wave? ›

    On 11 February 2016, the LIGO-Virgo collaborations announced the first observation of gravitational waves, from a signal (dubbed GW150914) detected at 09:50:45 GMT on 14 September 2015 of two black holes with masses of 29 and 36 solar masses merging about 1.3 billion light-years away.

    Is there gravity in the stratosphere? ›

    In the middle stratosphere (30–40 km), there is higher gravity wave activity near the equator in autumn in the middle stratosphere than in other seasons in 2020, and much less in 2021. The gravity wave activity is low (maximum 5 J kg1) compared to the lower stratosphere (maximum 10 J kg1).

    What are the waves in the stratosphere? ›

    This wave forcing of the flow is particularly important in the stratosphere, where this momentum deposition by planetary-scale Rossby waves gives rise to sudden stratospheric warmings and the deposition by gravity waves gives rise to the quasi-biennial oscillation.

    Are gravity waves everywhere? ›

    However, we do presume that many small gravitational waves are passing by from all over the Universe all the time, and that they are mixed together at random.

    What emits gravitational waves? ›

    The strongest gravitational waves are produced by cataclysmic events such as colliding black holes, supernovae (massive stars exploding at the end of their lifetimes), and colliding neutron stars.

    What do gravitational waves tell us about the universe? ›

    By tapping into this new source of information about the universe, gravitational wave astronomy might be able to solve some of the biggest puzzles in physics, including: how black holes form, how matter acts in extreme conditions, illuminating the nature of dark matter, and looking at the beginning of the universe long ...

    Can you hear gravitational waves in space? ›

    Astronomers have been able to “hear” the celestial hum of powerful gravitational waves, created by collisions between black holes, echoing across the universe for the first time.

    What is the rarest cloud? ›

    Nacreous clouds are some of the rarest clouds on the planet. They are a form of polar stratospheric cloud, which is a main culprit in chemical destruction of the ozone layer.

    How fast do gravity waves move? ›

    A gravitational wave is an invisible (yet incredibly fast) ripple in space. Gravitational waves travel at the speed of light (186,000 miles per second).

    What is the difference between a gravity wave and a ripple? ›

    Gravity waves, or gravitational waves, are essentially ripples in the fabric of space-time caused by accelerating masses. To put it simply, when an object with mass accelerates, the resulting gravitational force travels across space and time, creating waves of gravity that reach out infinitely at the speed of light.

    How do you explain gravity waves? ›

    “Gravitational waves are ripples in spacetime. When objects move, the curvature of spacetime changes and these changes move outwards (like ripples on a pond) as gravitational waves. A gravitational wave is a stretch and squash of space and so can be found by measuring the change in length between two objects.”

    What is the gravity in the atmosphere? ›

    What is the difference between a capillary wave and a gravity wave? ›

    The term 'gravity wave' is typically applied to wind-generated, periodic displacements of the sea surface, though nominally tsunamis are also gravity waves. A capillary wave is a wave travelling along the interface between two fluids, whose dynamics are dominated by the effects of surface tension.

    How do gravity waves affect tornadoes? ›

    According to Coleman, wave-storm interactions are very important. If a gravity wave hits a rotating thunderstorm, it can sometimes spin that storm up into a tornado.

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